Last giant impact on the Neptunian system: Constraints on oligarchic masses in the trans-Saturnian region

Context. Current models of the formation of ice giants attempt to account for the formation of Uranus and Neptune within the protoplanetary disk lifetime.Many of these models calculate the formation of Uranus and Neptune in a disk that may be several times the minimum mass solar nebula model (MMSN)....

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Detalles Bibliográficos
Autores principales:	Parisi, Mirta Gabriela, Valle, L. del
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2011
Materias:	Ciencias Astronómicas Planets and satellites: formation Planets and satellites: general
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/83996
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata Ver origen

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